Transcript Slide Title
Azimuthal correlation of hadrons in a partonic/hadronic transport model Guo-Liang Ma Background introduction Model introduction Analysis method Results and discussions Conclusion High Energy Nucleus-Nucleus Collisions initial state hadronic phase and freeze-out QGP and hydrodynamic expansion pre-equilibrium hadronization Physics: 1) Parton distributions in nuclei 2) Initial conditions of the collision 3) a new state of matter – Quark-Gluon Plasma and its properties 4) hadronization Di-hadron correlations pT(assoc) > 2 GeV/c Associated particles On away side: Hard associated particles → suppression pT(assoc) > 0.15 GeV/c Soft associated particles → enhancement Soft Associated particles on Away side (thermalization) What happens to a hard probe that traverses a colored medium? SOFTENED soften + broaden =?= thermalization near side away side thermalization??? BROADENED BROADENED SOFTENED Mach-like cone Structure Possible interpretations of mach-like cone structure Wake Effect or “sonic boom” Θemission= arccos (cs/c) hep-ph/0411315 CasalderreySolana,Shuryak,Teaney nucl-th/0406018 Stöecker Hep-ph/0503158 Muller,Ruppert nucl-th/0503028 A. K. Chaudhuri Cherenkov gluon radiation Θemission= arccos (1/n(p)) PRL 96, 172302 (2006) Koch, Majumder, X.-N. Wang Correlation of Jet with flowing medium hep-ph/0411341 Armesto,Salgado,Wiedemann AMPT model a multi-phase transport model (1) Default AMPT (2) Melt AMPT Mix-event Technique correlation signal in same event (2)Get respective background by mixing events in same centrality (3)Get correlation by removing background with ZYAM method 1/NtrigdNch/d (1) Get raw 530 520 510 500 490 480 470 4608 trig PT 3-6GeV/c ,PT asso 0.15-3GeV/c same event mix event 20-40% 6 20-40% 4 2 0 -1 0 1 2 3 4 5 Background Subtracted signal correlations from AMPT (3<pTtrigger<6GeV/c ,0.15<pTassoc<3GeV/c) 1/NtrigdN/d (1) ▲melt after Au+Au 200GeV (0-10%) hadron cascade 8 AMPT 0-10%,(3-6) x (0.15-3)GeV/c (2) ● melt 7 melt after hadron cascade before hadron melt before hadron cascade default after hadron cascade 6 cascade default before hadron cascade Star Data 0-5% (4-6) x (0.15-4)GeV/c factor=1.58 (3)◆ default 5 after hadron 4 cascade (4)★ default 3 before hadron 2 cascade 1 (5) ■ Star Data 0-5% (40 6)*(0.15-4)GeV/c -1 0 1 2 3 4 5 factor=1.58 (rad) Jet remnants character from AMPT associated Nhadron 16 2 10 (a) PT trig PT trig 14 3-6GeV/c (AMPT) near away 4-6GeV/c ( STAR data X factor=1.58) near away trig PT 4-6GeV/c (STAR data X factor=1.58) 0-5% away 0-5% near X 0.1 (b) -1 18 Au+Au 200GeV dNhadron/dP (GeV/c) 20 1 10 0 10 12 10 -1 10 8 6 trig PT -2 10 4 2 -3 3-6GeV/c (AMPT) 0-5% away 0-5% near X 0.1 10 0 2 4 6 8 10 12 0 1 2 (c) <pT>(Gev/c) 0.9 trig AMPT data PT 3-6GeV/c away trig STAR data PT 4-6GeV/c away (d) 1.0 <PT> (GeV/c) 1.0 0.8 0.7 PT trig PT trig 3 PT (GeV/c) impact parameter b (fm) 4 3-6GeV/c(AMPT) away 4-6GeV/c(STAR data) away 0.9 0.8 0.6 (0-10%) 0.7 0.5 -2 -1 0 - (rad) 1 2 0 2 4 6 8 10 impact parameter b (fm) 12 14 1.2 1.0 0.9 0.8 0.7 0.6 0.5 trig AMPT PT 2.5-4(GeV/c),PT associated 1-3.(GeV/c) melting after hadron cascade defaulting after hadron cascade trig associated experiment PT 2.5-4(GeV/c),PT 2-3(GeV/c) 0.4 0.3 0.2 1/NtrigdN/d 1/NtrigdN/d 1.1 2 4 6 8 10 impact parameter b (fm) 12 0-10% 0.3 0.2 0.1 -0.1 0.8 0.7 0.6 0.5 0.4 0.3 0.2 0.1 0.0 -0.1 0.7 0.6 0.5 0.4 0.3 0.2 0.1 0.0 -0.1 0.7 0.6 0.5 0.4 0.3 0.2 0.1 0.0 -0.1 0 1/NtrigdN/d spliting parameter D (rad) correlations in Au+Au 200GeV (2.5<pTtrigger<4GeV/c ,1<pTassoc<2.5GeV/c) 0.4 0-10% (2.5-4)X(1-2.5)GeV/c melt after hadron cascade factor=1/12 melt before hadron cascade factor=1/12 default after hadron cascade factor=1/5 default before hadron cascade factor=1/5 Phenix Data 0-5% factor=1.58 D 0.0 1/NtrigdN/d Mach-like cone Structure in AMPT model 0.5 10-20% (2.5-4)X(1-2.5)GeV/c melt after hadron cascade factor=1/5 melt before hadron cascade factor=1/5 default after hadron cascade factor=1/2 Phenix Data 10-20% faxtor=1.58 10-20% 20-40% (2.5-4)X(1-2.5)GeV/c melt after hadron cascade factor=1/5 melt before hadron cascade factor=1/5 default after hadron cascade factor=1/2 Phenix Data 20-40% factor=1.58 20-40% 40-90% (2.5-4)X(1-2.5)GeV/c melt after hadron cascade factor=1/4 melt before hadron cascade factor=1/4 default after hadron cascade factor=1/2 Phenix Data 60-90% factor=1.58 40-90% 1 (rad) 2 3 Three-particle correlations in AMPT mix-event technique background subtracted 3-particle correlation signal Three-particle correlation density 3-particle correlation density definition: d 2N d1d2 d1d2 region d d 1 2 region 70 open: melt before 60 full: melt after 40 30 ratio center deflected cone near near-away 50 (a) 20 10 0 0 100 200 Npart 300 2.6 (b) 1.16 2.4 1.12 2.2 1.08 1.04 2.0 1.00 1.8 1.6 open: melt before 1.4 full: melt after 1.2 center/deflected center/cone 1.0 0 open: melt before full: melt after deflected/cone 0 100 200 300 100 N 200 part 300 Parton cascade effect on 2- and 3particle correlation (1)hadron cascade mechanism also can produce 2- and 3-particle correlation, but it can not give big enough splitting parameters. (2) the parton cascade mechanism is essential for describing the amplitude of experimental mach-like structure Conclusion 1) Di-hadron correlations can be produced by a multiphase transport model(AMPT). 2) Mach-like structure is born in the partonic process and further developed in hadronic rescattering process. 3) hadron cascade mechanism can produce dihadron correlation, but it can not give big enough splitting parameters. 4) Cone , deflected and center 3-particle correlations all exist in the central Au+Au collisions, however center 3-particle correlation become more dominant with the decreasing of Npart . Thank you